Descubre y comparte nuestro conocimiento público

Se han encontrado 23 recursos

Resultados de búsqueda

Article 2016

Autor: Gonzalez, O.A. Gadotti, D.A. Debattista, V.P. Rejkuba, M.de Valenti, E. Zoccali, M. Coccato, L. Minniti, D. Ness, M.

Context. Our view of the structure of the Milky Way and, in particular, its bulge is obscured by the intervening stars, dust, and gas in the disc. While great progress in understanding the bulge has been achieved with past and ongoing observations, the comparison of its global chemodynamical prop...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/836

Repositorio Universidad Andrés Bello
Enlace permanente

Gonzalez, O.A. ,  Gadotti, D.A. ,  Debattista, V.P. ,  Rejkuba, M.de ,  Valenti, E. ,  Zoccali, M. ,  Coccato, L. ,  Minniti, D. ,  Ness, M. ,  [Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE] ,  Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE
Article 2016-07

Autor: Gran, F. Minniti, D. Saito, R. K. Zoccali, M. Gonzalez, O. A. Navarrete, C. Catelan, M. Contreras Ramos, R. Elorrieta, F. Eyheramendy, S. Jordán, A.

Context. The VISTA Variables in the Vía Láctea (VVV) is a near-IR time-domain survey of the Galactic bulge and southern plane. One of the main goals of this survey is to reveal the 3D structure of the Milky Way through their variable stars. In particular, enormous numbers of RR Lyrae stars have b...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/2786

Repositorio Universidad Andrés Bello
Enlace permanente

Gran, F. ,  Minniti, D. ,  Saito, R. K. ,  Zoccali, M. ,  Gonzalez, O. A. ,  Navarrete, C. ,  Catelan, M. ,  Contreras Ramos, R. ,  Elorrieta, F. ,  Eyheramendy, S. ,  Jordán, A. ,  [Mapping the outer bulge with RRab stars from the VVV Survey] ,  Mapping the outer bulge with RRab stars from the VVV Survey
Article 2016-03

Autor: Valenti, E. Zoccali, M. Gonzalez, O. A. Minniti, D. Alonso-García, J. Marchetti, E. Hempel, M. Renzini, A. Rejkuba, M.

We present the first stellar density profile of the Milky Way bulge that reaches latitude b = 0 degrees. The profile was derived by counting red clump stars within the colour-magnitude diagram that was constructed using the new PSF-fitting photometry from VISTA Variables in the Via Lactea (VVV) s...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/3974

Repositorio UNAB
Enlace permanente

Valenti, E. ,  Zoccali, M. ,  Gonzalez, O. A. ,  Minniti, D. ,  Alonso-García, J. ,  Marchetti, E. ,  Hempel, M. ,  Renzini, A. ,  Rejkuba, M. ,  [Stellar density profile and mass of the Milky Way bulge from VVV data] ,  Stellar density profile and mass of the Milky Way bulge from VVV data

Selecciona los documentos para visualizarlos

Nombre del archivo Ver recurso
Marcar todos
Limpiar todo